Solar Images Monday, 30 June 2025
‹ 29.06.2025 2025 01.07.2025 ›Photosphere sunspot drawing and RDS evaluation
- Time
- 11:45 UT
- Observer
- Süleyman FİŞEK
- g
- 13
- f
- 53
- R
- 183
- Seeing
- 3 / 5
Sunspot groups and observation details →
Sunspot groups (from the drawing)
RDS data file (.gzd)
[Gözlem] Tarih=30.06.2025 Saat=11:45 Gözlemci=Süleyman FİŞEK KontrolEden= Durumaçısı=-2.83 Enlemaçısı=2.81 Boylamaçısı=214.7 Boylamfark=0 GKalite=3 GDurum=G.T , H.S Kuzeyaçısı=-0.5 Sırano=20286 AyRasatNo=29 RasatÖnceki=29.06.2025 RasatSonraki=1.07.2025 [Leke Grupları] Grupsayısı=13:5:8 LekeSayısı=53:31:22 RölatifSayı=183:81:102 01=HS_ 01 +17.833 +84.575 299.275 -1.000 0000 0 +18.369 +86.588 +17.298 +82.561 02=AX_ 01 +14.815 +48.541 263.241 -1.000 0000 0 +14.815 +48.541 +14.815 +48.541 03=DSI 14 +13.393 +01.779 216.479 +0.000 0000 0 +16.840 +06.597 +10.702 -03.400 +13.393 +06.397 +13.393 -02.840 04=HS_ 02 +21.374 -41.154 173.546 -1.000 0000 0 +22.508 -40.100 +20.240 -42.298 05=DSC 13 +02.446 -45.917 168.783 +0.000 0000 0 +04.150 -42.545 +00.878 -49.289 +02.446 -42.745 +02.446 -49.890 06=AX_ 01 -13.455 +61.915 276.615 -1.000 0000 0 -13.455 +61.915 -13.455 +61.915 07=DSC 06 -27.616 +15.857 230.557 +0.000 0000 0 -26.285 +18.830 -28.948 +12.884 -27.616 +18.630 -27.616 +13.840 08=HS_ 01 -13.999 -17.304 197.396 -1.000 0000 0 -13.667 -16.889 -14.331 -17.718 09=DSI 06 -17.556 -27.582 187.118 +0.000 0000 0 -16.515 -25.165 -18.597 -29.999 -17.556 -25.365 -17.556 -29.799 10=CSI 04 -04.578 -34.307 180.393 +0.000 0000 0 -03.773 -31.340 -05.383 -37.580 -04.578 -31.234 -04.578 -37.380 11=AX_ 01 -08.150 -44.819 169.881 -1.000 0000 0 -08.150 -44.819 -08.150 -44.819 12=HS_ 02 -16.401 -77.396 137.304 -1.000 0000 0 -15.862 -75.498 -16.940 -79.494 13=AX_ 01 -11.767 -77.481 137.219 -1.000 0000 0 -11.767 -77.481 -11.767 -77.48120250630.gzd
Chromosphere (H-α) FITS frames
The images are made automatically with a fixed, gentle rule: uneven illumination and most of the limb darkening are removed, and the brightness is shown on a linear scale (no sharpening); prominences get their own scale outside the limb. Frames are ordered by sharpness (seeing); frames without the Sun (darks, bias) come last. Method →
2025/20250630_sf · SF · 6 frames · 128.6 MB · 11:51:59–11:55:57 UT
Coronado H-α animations from frame sequences
No Coronado observation for this day.








